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Table 3

Dust properties summary of the targets under study I.

Comet Emission Active areas Size distribution Size distribution Maximum nucleus Obliquity Argument of subsolar
pattern1 location (°) rmin,rmax (cm) δ min , δ max radius (km) (°) meridan at perihelion (°)

30P/Reinmuth 1 Ani (50%) –30 to +30 10-4, 3.5 –3.35, –3.18 3.92 107 3 1333
78P/Gehrels 2 Iso (100%) 10-4, 3.0 –3.40, –3.05 3.6
115P/Maury Ani (70%) –20 to +60 10-4, 4.0 –3.13, –3.05 4.0 25 280
118P/Shoemaker-Levy 4 Iso (100%) 10-4, 3.0 –3.20, –3.05 2.44
123P/West-Hartley Iso (100%) 10-4, 2.5 –3.32, –3.15 2.05
157P/Tritton Ani (70%) –30 to +30 10-4, 3.0 –3.35, –3.15 1.6 10 150
185P/Petriew Iso (100%) 10-4, 6.0 –3.60, –3.00 5.7
P/2011 W2 (Rinner) Iso (100%) 10-4, 2.5 –3.20, –3.15 2.2

Notes.

(1)

Iso = Isotropic ejection; Ani=Anisotropic ejection;

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